Is this a way to move faster than c?

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In summary: But just like with a globe, without outside space we would not be able to measure distances or angles. In summary, if you are trying to move a galaxy away from Earth faster than the speed of light, you will not be able to do so because the laws of physics will keep it from happening.
  • #106
bcrowell said:
I would definitely argue that Born-rigid bodies are useless. For a good discussion of this, see Ø. Grøn, Relativistic description of a rotating disk, Am. J. Phys. 43 869 (1975). In section IV, he shows that giving an angular acceleration to a Born-rigid body is a kinematical impossibility.
Born rigid bodies are not useless for linear acceleration and could in principle exist and be accelerated with Born rigid motion. In the case of a Born rigid disk, we could give it Born rigid angular acceleration, if we relax the constraint that the radius must remain constant. I guess a Born rigid ring would be more appropriate in that case, which could be spun up to a given angular velocity while the distance between adjacent points on the ring remains constant from the point of view of observers on the ring, if the radius of the ring is allowed to shrink by the appropriate amount as the ring is spun up. In the case of a ring that circles the closed universe, there is no requirement to give it angular velocity. Sure the distance between adjacent observers on the ring is increasing as the universe expands, so that the observers appear to be moving relative to each other, but there is no overall angular motion imparted to the ring.
 
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  • #107
This is an attempt at an counter argument to the "we can ignore all the mass in the universe that is not inside the sphere under consideration" argument, when calculating effective relative gravitational potentials in a homogeneous universe. Let's call this second argument the "effective sphere" argument for brevity.

Consider two stationary observers, A and B a distance 2r apart in a static(not expanding) infinite, homogeneous density, isotropic universe. To calculate the redshift of a signal from B as observed by A, we consider a sphere of radius r centred on A and ignore all the mass outside this hypothetical sphere. Now let us say that a star near B is visible from A. B measures the characteristic emission spectrum of excited hydrogen locally as w. The effective sphere argument predicts that A at the centre of his effective sphere, sees B at a higher gravitational potential and A measures the received wavelength to be blue shifted relative to the emitted wavelength measured by B locally. Similarly B measures the received light from A's star to be blue shifted relative the emitted wavelength measured by A.

Now a third observer exactly half way between A and B observes that both A and B are at the surface of the sphere centred on C and that the wavelength of the signal received by A will have exactly the same wavelength as the emission signal measured by B when it was emitted. This is a direct contradiction to the earlier statement that A measures the signal sent from B to blue shifted. Therefore, it would seem that the effective sphere argument and being able to ignore the rest of the universe argument is flawed.

My argument is based on a non expanding universe and I guess it is possible that some effect due to expansion causes some sort of cancellation of terms and allows us to ignore material external to the effecitve sphere, but this would be very coincidental and precise expansion (or maybe it is not coincidental and the two things are related)?

Counter-counter-arguments to my counter-argument are welcome :wink:
 
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  • #108
kev said:
It is true that in GR there are various coordinate systems and different ways of defining distance but do you agree that if we attach a wire to a distant galaxy (not necessarily superluminal) then there should be an unambiguous answer to the velocity of the end of the wire that passes right by us, even if we are having trouble calculating exactly what it would be at the moment?
Absolutely not. For example, you could use this method to get a nonzero answer for the Milky Way's velocity relative to itself, if the wire passed all the way around a closed universe. That seems like a clear ambiguity to me. There are all kinds of issues with the dynamics of the wire, the initial conditions, etc., which make it unclear whether the wire can be constructed and put in place, whether it transmits useful information, etc. These aren't just difficulties with knowing how to do certain calculations; they're signs that the rope's intended purpose in the OP's thought experiment is fundamentally meaningless. It's similar to describing a thought experiment designed to determine an observer's velocity with respect to the ether. That velocity is meaningless to talk about.

kev said:
In other words if the measure the redshift of the distant galaxy to be z then we should be able to say that that the velocity of the end of the wire nearest us would be v(z) where v is a function of z. This is the most unambiguous and intuitive definition of the velocity of the distant galaxy relative to us that I can think of.
No, that doesn't work either. There is no unambiguous way to resolve the redshift into gravitational and kinematic parts. Two good papers on this are [Bunn] and [Francis]. If you prefer to call it 100% kinematic, then Bunn shows you can do that. If you prefer to say that part of it is gravitational, and space is expanding, then Francis shows you can do that.

kev said:
I really like this idea. I think it would be a very good basis for any objective analysis of the problem at hand, but I have a slightly different operational definition to yours.
It would be very interesting to figure out if there is a unique, self-consistent way of extending the idea of Born-rigidity from SR to GR. In SR there are various types of limitations on Born-rigidity, such as the inability to perform angular accelerations, and it took decades after Born's initial definition for these limitations to be clearly understood. If one doesn't understand those limitations, one can use Born-rigidity to prove all kinds of paradoxes in SR. Personally, I strongly doubt that there is any useful or interesting way to generalize Born-rigidity to GR. If you think such a generalization might be helpful in the current thread, then probably the first thing to do would be to search the literature. Maybe it's been shown to be impossible to generalize, or it's been shown that the generalization is non-unique, or every proposal for generalizing it has been shown to be non-self-consistent. But I think that if anyone wants to use Born-rigid objects in the present discussion, the burden of proof should be on them to demonstrate that the idea of Born-rigidity in GR has been studied and found to be meaningful. Without any such evidence, I'm not willing to accept any argument based on Born-rigidity, because it's just too easy to come up with obviously paradoxical examples, such as wrapping a Born-rigid ring around a closed spacelike geodesic in a closed cosmology.

kev said:
The secondary question is, will observers that are are at constant ruler and radar distance from each other, measure a redshift in signals sent to each other, if the distances and travel times are cosmologically significant?
Hmm...you're trying to substitute notions like constant-ruler-distance and constant-radar-distance for the idea of a wire, but I don't think that helps. A ruler is just a wire by another name, or possibly a wire with a slightly different set of dynamical properties. The notion of constant radar distance is frame-dependent. Suppose A and B determine themselves to be at constant radar distance from one another. Observer C, at a cosmologically distant location, says that A and B are both accelerating, and therefore their time-dilation factors are changing over time. C says that the round-trip radar signals between A and B are actually taking different amounts of time.

[Bunn] http://arxiv.org/abs/0808.1081v2
[Francis] http://arxiv.org/abs/0707.0380v1
 
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  • #109
Ich said:
If it makes your head hurt, start with simpler things, get your head around them, and then advance to higher levels of complexity.
If you had given a self-consistent definition of what you meant by the generalization of Born-rigidy to GR, then it would have been legitimate to challenge me to wrap my head around your definition. But you haven't given a valid definition. I've shown that your definition is not self-consistent, and I've said that trying to fix your definition makes my head hurt. If you want to come up with a definition that is self-consistent, then it's up to you to do that, not me.
 
  • #110
kev said:
I think closed universes are a bit messy and current cosmological observations can not rule out a flat or open universe. Personally, I hope advanced measurements will rule out the closed case and make that mess go away.
The paradoxes are just easier to pose in the case of a closed universe. I've given lots of examples in this thread that don't involve a closed universe. The underlying issue is that relative velocities of cosmologically distant objects are not well defined. This is a standard part of the interpretation of GR, and it applies to both closed and open universes.

kev said:
Consider two galaxies a distance (x) apart on the surface of sphere of radius (r) that represents the topology of a closed universe. Normally we would say the the gravitational attraction between the two points is proportional to GM/x^2. In the closed universe we would have to say there is an additional force that goes all the way around the universe the long way, with magnitude GM/(2*PI*r -x)^2 that acts to pull the galaxies apart. That means we would have to reformulate the equation for gravitational attraction.
Einstein did formulate the equation for gravitational attraction. That's what GR is.

kev said:
This of course assumes that the universe has existed long enough for the two points to become aware of their effective mirror image in the closed universe. As I said, closed universes are a bit messy and I hope they go away soon :-p. Some cosmologists have actually looked at the patterns in the CMB to see if there are repeating patterns in opposite parts of the sky suggesting a closed universe and failed to find any evidence for the closed universe idea, using that method.
I think the observations you have in mind were something different. There's the possibility that the universe has a nontrivial topology, and there have been searches for evidence of that. For instance, you can have a universe that looks like the flat FLRW solution locally, but has the topology of a strangely connected soccer ball or something. Even in closed universes with a zero cosmological constant, I believe you can only see the back of your own head through a telescope after a certain point in time.
 
  • #111
I mentioned the internal Schwarzschild non-vacuum solution earlier. In its simple form (no linear or angular motion) it can be expressed as:

[tex]d\tau_r^2 = dt^2 \left(\frac{3}{2} \sqrt{1-\frac{2GM}{c^2 a}} - \frac{1}{2}\sqrt{1-\frac{2GMr^2}{c^2 a^3}} \right) [/tex]

where a is the surface radius of the gravitational body and r is location of a stationary clock that measures proper time [itex]d\tau_r[/itex] inside the body (r<=a) and M is the total mass of the gravitational body. Outside the gravitational body is considered to be a vacuum and is covered by the external Schwarzschild solution.

For uniform density (p) using the simple formula of total mass divided by total volume so that:

[tex]p=\frac{3M}{4\pi a^3} [/tex]

and using a factor K defined as:

[tex]K = \frac{8\pi G}{3c^2} [/tex]

the internal solution can now be expressed as:

[tex]dt_r^2 = dt^2 \left((3/2)\sqrt{1-pKa^2} - (1/2)\sqrt{1-pKr^2}\right) [/tex]

If we consider the special case of a clock located at the centre of the body the proper time of this clock is given by:

[tex]d\tau_0^2 = dt^2\left( (3/2)\sqrt{1-pKa^2} - 1/2\right) [/tex]

The ratio between clock rates of a clock located at r and another clock located at the centre of the body is then given by:

[tex]\frac{dt_r}{dt_0} = \left(\frac{3\sqrt{1-pKa^2} - 2\sqrt{1-pKr^2}}{-1+3\sqrt{1-pKa^2}}}\right)^{1/2} [/tex]

Now the "effective sphere" argument for an infinite universe of constant density means we can ignore all mass at a greater radius than a from the centre and so we can treat the external as a vacuum and declare the internal Schwarzschild metric as a valid way to anlayse this effective sphere.

Now if we carry out the calculate the ratio of the clock rate ratios for a>r and then repeat the calculation for a=r, (effectively removing the shell with internal radius r and external radius a), we see that the ratio between the clock rates at the centre and r increases. This suggesting that the red or blue shift measured between points at the centre and at r is dependent on the mass in spherical shells at radii greater than r, suggesting that our initial assumption that we can treat mass external to the effective sphere as vacuum, is flawed. In fact if a is sufficiently large the clock at the centre stops and after that the clock at the centre starts running backwards or becomes imaginary and the region presumably collapses in on itself and becomes a black hole. To me, it is more satisfactory to consider all points in a homogeneous infinite universe to be at equal gravitational potential at any given time, and in this case, the only way effective gravitational potentials can arise between points, is by by temporal changes in potential in an expanding universe.
 
  • #112
bcrowell said:
If you had given a self-consistent definition of what you meant by the generalization of Born-rigidy to GR
What I meant with a generalizsation of Born-rigidity to GR? That's completely your idea.
What I meant to do, and I explicitly said so, is to give the definition of a rope in the context of this thread some rigor. Which I did.
Born rigidity was merely an analogy, because you flamed against pre-arranged motion.
And I applied the definition explicitly to open topologies only.
And I said
Ich said:
I'll have to think more about the closed topology case, which is more complicated. But I think the open case is interesting enough for now.
Which means: I have no idea how to generalize the notion to arbitrary topologies, and it makes my head hurt if I think about it. And I'll think about it later.

bcrowell said:
If one doesn't understand those limitations, one can use Born-rigidity to prove all kinds of paradoxes in SR. Personally, I strongly doubt that there is any useful or interesting way to generalize Born-rigidity to GR.
etc. etc.
Calm down. You are talking about generalizations of Born rigidity, not I. I'm talking about the OP's rope. In an open topology.

If you're interested in that rope thing, as you indicated, then I'm sure it's worthwile for you to follow the definition I gave - even if you could call it original research, as I never bothered to find sources for it. Because the principles are not too complicated for a forum discussion, and the results are easy to check analytically with the Milne/de Sitter models.
 
  • #113
kev said:
The effective sphere argument predicts that A at the centre of his effective sphere, sees B at a higher gravitational potential and A measures the received wavelength to be blue shifted relative to the emitted wavelength measured by B locally. Similarly B measures the received light from A's star to be blue shifted relative the emitted wavelength measured by A.
No.
If all observers are to stay at fixed distances, at least some of them have to undergo proper acceleration. Either A, or B, or both. It's your say.
If you choose one which is free falling, this one is the hub of the world. All red- or blueshifts are directed towards it.
Check it with Newtonian gravity, interior Schwarzschild is definitely an overkill.
 
  • #114
I am not quite sure I understand you here. The stationary observer low down sees a gravitational redshift of the signal from higher up (basically because his clock is running slower)
Blueshift, of course.
Not sure why you said "observer losing speed during the light travel time" unless you meant he had an effective velocity away the source initially
Yep, I was talking about comoving observers. Only they are interchangeable.
I think it would be a very good basis for any objective analysis of the problem at hand, but I have a slightly different operational definition to yours.
From what I can tell, your definition is exactly the one I used, as long as you define "radar distance" to be the back and forth light travel time.
There's only one thing you omit, and it throws you off the curve in your later analysis: You have to pick an origin, the preferred point without proper acceleration.
Now if I use the argument of "temporal differences of gravitational potential" that I introduced earlier, then I have to consider how that will affect the radar distance over time.
Don't use it.
In other words, non-zero redshift does not imply non-zero relative motion using this idea.
This is definitely true, and it's the reason why I defined "constant distance" by a two-way measurement.
But the redshift has nothing to do with your alleged "temporal potential". It's a simple spatial potential, centered at the origin. All those redshifts either point toward it, or away from it. There's nothing reciprocal, and in fact it's irrelevant whether there is expansion or contraction. The only thing that counts is the local matter (and pressure) density.
In the Schwarzschild example, signals from a stationary source lower down, redshift because they come from a PLACE where gravitational potential is lower, while in the temporal gravitational potential example, signals from a stationary source redshift, because they come from a TIME when gravitational redshift was lower.
Yes, I understood. This doesn't work. The redshift indeed comes from a PLACE where the potential is lower.
The primary question is will a very distant observer at the end of very long chain of observers at rest wrt us, ever see galaxies that are near them, but at rest with the Hubble flow, moving at greater than the speed of light relative to themselves and I am pretty sure most people here would agree that the answer is no.
I already said that there are two (or three, depending on how you count) different possibilities for the end of the chain:
1) It goes asymptotically to v=c in an infinite distance. That's the Milne model with its coordinate singularity.
2) It ends in a horizon, where the chain breaks. That's the de Sitter model, which is like an inverse black hole.
3) It ends abruptly in the Big Bang. These are the matter-containing models, where at one time everything is ok - if a bit frantic, and in the very next moment everything falls toward the end of the chain at light speed.
This moment is, of course, the Big Bang singularity, and not part of the manifold we're considering.

One thing is ubiquitous: The "rope simultaneity" goes further and further back in time with increasing distance, if compared with FRW time. If there is a Big Bang (all models except de Sitter), the end of the rope will be there, either in a finite (models with matter) or infinite (Milne/empty model) comoving distance.
 
  • #115
BTW, I'm away for a week now. Maybe we can contiue this discussion later.
 
  • #116
kev said:
Now the "effective sphere" argument for an infinite universe of constant density means we can ignore all mass at a greater radius than a from the centre and so we can treat the external as a vacuum and declare the internal Schwarzschild metric as a valid way to anlayse this effective sphere.
I don't think this works. Birkhoff's theorem implies that if you have a spherical cavity in a spherically symmetric universe, you can ignore the external mass, and the spacetime inside the cavity has to be Minkowski. It doesn't tell you anything about the case where there is no spherical cavity. It's different from the Newtonian-gravity shell theorem, because GR isn't linear like Newtonian gravity. Therefore you can't take just any old spherically symmetric mass distribution, break it down into concentric shells, and sum the fields made by the shells.

kev said:
To me, it is more satisfactory to consider all points in a homogeneous infinite universe to be at equal gravitational potential at any given time, and in this case, the only way effective gravitational potentials can arise between points, is by by temporal changes in potential in an expanding universe.
As I've been pointing out since #67, you can't analyze cosmological solutions using a gravitational potential. You need a static spacetime in order to define a gravitational potential. There is a good discussion of this in Rindler, Essential Relativity, 2nd ed., section 7.6. If cosmological solutions could be described by a gravitational potential, then you would be able to resolve cosmological red-shifts into unambiguously defined kinematic and gravitational terms. But this is impossible, as discussed in the references in #14.
 
  • #117
Ich said:
Blueshift, of course.
Yes, of course. I have corrected my typo in the original post. Thanks.
Ich said:
From what I can tell, your definition is exactly the one I used, as long as you define "radar distance" to be the back and forth light travel time.
Yep, that is what I meant by radar distance.
Ich said:
There's only one thing you omit, and it throws you off the curve in your later analysis: You have to pick an origin, the preferred point without proper acceleration.
I find this an odd statement. In a FLRW universe, most significant objects are at rest with the Hubble flow and nothing has proper acceleration in the cosmological sense. When we see a distant galaxy moving away from us at some great velocity and even if we acknowledge dark energy or the cosmological constant, neither the distant galaxy or ourselves have proper acceleration with respect to each other, not the kind you can measure with an accelerometer anyway. Both the distant galaxy and ourselves will appear to be approximately at rest with respect to the CMBR.

Ich said:
Don't use it.
I was hoping for a more detailed counter argument than "don't use it" and "forget about it" to my argument. :-p

Ich said:
But the redshift has nothing to do with your alleged "temporal potential". It's a simple spatial potential, centered at the origin. All those redshifts either point toward it, or away from it. There's nothing reciprocal, and in fact it's irrelevant whether there is expansion or contraction. The only thing that counts is the local matter (and pressure) density.
Is it relevant if there is neither expansion nor contraction? (i.e a static universe). I can see a spatial potential in a finite universe where clearly objects "near the edge" will have a different potential to objects near the centre, but in an infinite universe, there is no such thing as a centre or a near the edge. You have not made it clear (to me anyway) whether you are talking baout finite or infinite models.

Ich said:
Yes, I understood. This doesn't work. The redshift indeed comes from a PLACE where the potential is lower.
I still don't get this. In an infinite homogeneous universe, WHERE is this PLACE with a lower potential?

Ich said:
I already said that there are two (or three, depending on how you count) different possibilities for the end of the chain:
1) It goes asymptotically to v=c in an infinite distance. That's the Milne model with its coordinate singularity.
Yep, that makes sense, and if you can only construct the chain at a velocity that is less than the speed of light, the chain will never catch up with the edge of the visible universe. However, the Milne model has obvious limitations because it does into take into account the GR effects of all that moving matter and energy in the universe.

Ich said:
2) It ends in a horizon, where the chain breaks. That's the de Sitter model, which is like an inverse black hole.
One thing we have not really addressed in this thread is the physical stress that a rope would be subjected to, when it joins two distant galaxies that are at rest with respect to each other. Just how much drag does the Hubble flow apply to an object that is not at rest with the Hubble flow? I would suggest none or very little. It is our experience that an object with a peculiar local velocity continues to move with velocity and is not subjected to any drag bringing it to rest with the CMBR.

Ich said:
3) It ends abruptly in the Big Bang. These are the matter-containing models, where at one time everything is ok - if a bit frantic, and in the very next moment everything falls toward the end of the chain at light speed.
This moment is, of course, the Big Bang singularity, and not part of the manifold we're considering.

One thing is ubiquitous: The "rope simultaneity" goes further and further back in time with increasing distance, if compared with FRW time. If there is a Big Bang (all models except de Sitter), the end of the rope will be there, either in a finite (models with matter) or infinite (Milne/empty model) co-moving distance.
I agree with this conclusion, but it makes your head hurt to think of a wire physically connecting here and now at one end and the big bang at the other end. Ouch!

Ich said:
BTW, I'm away for a week now. Maybe we can continue this discussion later.
Looking forward to your return. Have a pleasant trip! :smile:
 
  • #118
I have been gone for a few weeks...

What are you positing moves faster than light? Light itself? Does c refer to a hard 300,000,000 km/sec or just the speed of light, whatever that is. Light moves slower than 300 million m/sec traveling through media.

How does adding proper times up over long distances get you faster than light speed as presented earlier? How do non linear coordinates get you faster than light speed? Minkowski coordinates have no central frame of reference, so how is that possible in any coordinate system. After all, anything you chose as "central" would be arbitrary.

Einstein's "nothing faster than c" is a hypothesis. Has it ever been disproven? Can anyone give a mathematical example of how one could travel faster than light that makes any sense?

Two simultaneous events in the same frame of reference are spacelike separated and one cannot get from A to B "in tmie" Has that ever happened before?

This is pretty damn confusing. but I can understand that light speed does not have to be constant, now does it?
 
  • #119
Looking forward to your return. Have a pleasant trip!
Thanks. We've been to http://www.ferienhof-rosenlehner.de/bauernhof.html" , but sadly there were not enough possibilities for my youngest son to practice his skills as a farmer - which he is determined to become. Still, a beautiful place.

Ich said:
There's only one thing you omit, and it throws you off the curve in your later analysis: You have to pick an origin, the preferred point without proper acceleration.
I find this an odd statement. In a FLRW universe, most significant objects are at rest with the Hubble flow and nothing has proper acceleration in the cosmological sense. When we see a distant galaxy moving away from us at some great velocity and even if we acknowledge dark energy or the cosmological constant, neither the distant galaxy or ourselves have proper acceleration with respect to each other, not the kind you can measure with an accelerometer anyway. Both the distant galaxy and ourselves will appear to be approximately at rest with respect to the CMBR.
Everything you say is true, but IIRC we've been talking about the chain of observers who are mutually at rest in this case. Such observers are not comoving, and if there is gravity, all but one will experience proper acceleration.
You'll have to define an origin for that chain. The origin will be moving inertially, all other elements generally won't.
Ich said:
Don't use it.
I was hoping for a more detailed counter argument than "don't use it" and "forget about it" to my argument.
I thought I did, in the subsequent paragraph.
The redshifts in a chain of "stationary" observers are not reciprocal, as they should be if we're talking about a change in time only.
Further, they are independent of expansion or contraction. They only depend on the local mass density, not its time derivative.
Is it relevant if there is neither expansion nor contraction? (i.e a static universe). I can see a spatial potential in a finite universe where clearly objects "near the edge" will have a different potential to objects near the centre, but in an infinite universe, there is no such thing as a centre or a near the edge. You have not made it clear (to me anyway) whether you are talking baout finite or infinite models.
I'm talking about infinite models, too. But if you want to use the well-known potential, you'll have to pick an origin and use quasistatic coordinates in its vicinity. In expanding FRW coordinates, there is no potential.
Ich said:
Yes, I understood. This doesn't work. The redshift indeed comes from a PLACE where the potential is lower.
I still don't get this. In an infinite homogeneous universe, WHERE is this PLACE with a lower potential?
The place with extreme (max or min) potential is just where you pick the origin of the chain of stationary observers. Pick another origin, and there will be a different potential. But it doesn't matter for your calculations.

But your idea of a "temporal potential" has some merit: In FRW coordinates, the scale factor is the equivalent of a potential in static coordinates.
The former is a scale of position as a function of time, while the latter is a scale of time as a function of position.
The former defines changes in momentum, the latter defines changes in energy.
That said, the word "potential" usually does not refer to somthing like a scale factor, and I'm not sure if this would be a good idea.
But ok, there are the complementary pairs: time - position, energy - momentum, potential - scale factor.

Just how much drag does the Hubble flow apply to an object that is not at rest with the Hubble flow? I would suggest none or very little.
Right. The Hubble fow in itself is a property of a family of observers, not a property of spacetime. It cannot possibly exert some kind of drag (usual disclaimer for nitpickers:, except for higher order corrections in the presence of mass).
For local physics, it is irrelevant whether there is outward, inward, or no Hubble flow at all. The Hubble flow is then nothing but the average motion of galaxies.
It is our experience that an object with a peculiar local velocity continues to move with velocity and is not subjected to any drag bringing it to rest with the CMBR.
Nope. Peculiar velocities tend to die out, but that's a sorting effect, not a force or drag. If something has peculiar velocity, it will simply move to a place where it hasn't.
I agree with this conclusion, but it makes your head hurt to think of a wire physically connecting here and now at one end and the big bang at the other end. Ouch!
Well, it's not so painful if you remember that the wire is not exactly a "physical connection". In the wire's frame, all its components are spacelike separated, and the supposed fate of its ends is really irrelevant for what's happening here and now.
 
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  • #120
stevmg said:
I have been gone for a few weeks...

What are you positing moves faster than light? Light itself? Does c refer to a hard 300,000,000 km/sec or just the speed of light, whatever that is. Light moves slower than 300 million m/sec traveling through media.

As far as the original post my way of thinking was, I know (in my own way of understanding things) that nothing with rest mass can propagate at or faster than the speed of light in any medium. However, does that mean that nothing can move away from me faster than the speed of light?

According to GR, the universe is expanding and thus there are distant objects that are moving away from me at the speeds greater than the speed of light.

If so, is it then possible to use this fact to show that, although nothing can propagate through any medium faster than the speed of light, information could still be passed on faster than the speed of light.

Again, the thought process was although nothing can travel faster than c in any medium I know of, if the medium was moving away from me as well (or expanding as space seems to be.) then it seems to be possible, at least in theory.

Now I don't pretend to understand all of the very good and detailed answers given but as far as can make out, there has been no conclusive proof of this either way. ( I think!) :confused:
 
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  • #121
From all this all I can gather is that in order to exceed the speed of light. time-space itself must expand. Again, it has never been shown that light speed cannot differ from 300 X 106 m/sec but nothing has shown that it does differ from that other than traveling through media.

Even if you think about it the searchlight paradigm fails. Think of a circular sprinkler system. The fastest any of the particles are moving laterally is the linear speed they had when they left the sprinkler.

Proper time doesn't add up either. At least I would like to see some simple mathematical model of how this could create transmission greater than light speed.

From Fiddler on the Roof there is an analogous situation explained: "If I were the Tsar, I would be richer than the Tsar!"
"How so?"
""I would have all the wealth and power of the Tsar, and...
.
.
.
.
.
I would do a little teaching on the side!"
 
  • #122
I can not see that space is curved
 
  • #123
If we talk about how to moove faster then speed of light, then we must consider which law has given this restriction , If we prove that law to be wrong ( I mean if we prove special theory of relativity wrong) then it could be I have tried to proove that to know visit http://sallubhai007.blogspot.com
 
  • #124
sallubhai007 said:
I can not see that space is curved

That's because what your seeing isn't where you think it is.
 
  • #125
we can refer shape to only material thing like a ball and we can not refer shape to non-material things like electric field , magnetic field etc ,althou we know that they exist like that space is also a non-material thing then why we talk about its shape imean its curve
 
  • #126
So, what's the consensus? Appears that there is no proof that we can move faster than c (=300 million m/sec.) In fact, there is no proof that c is constant everywhere in this or another universe, just local to what we know.
 
  • #127
stevmg said:
So, what's the consensus? Appears that there is no proof that we can move faster than c (=300 million m/sec.) In fact, there is no proof that c is constant everywhere in this or another universe, just local to what we know.

According to general relativity (and ignoring the hypothetical, but very unlikely, possibility that tachyons might exist), nothing can overtake a photon that is traveling along the same route.

The numerical value of the speed of a photon depends on the coordinate system you measure it in. If you measure it locally, using a "local ruler" x and "local clock" t, you will always get dx/dt = c (=299792458 m/s exactly) no matter where you are in the Universe or how you are moving. But if you try to measure the speed of some light a distance away from yourself, you may well get a different numerical value. This is due to spacetime curvature. An analogy is that cartographers can accurately draw a scale map of an area a few miles across, but if you try to map a thousand miles of the Earth's surface on a flat piece of paper, the map could be very accurately to scale at the centre of the map, but distorted in angle or distance near the edges. This is what happens in relativity, long-distance measurements can get distorted.

As for the expanding Universe, the simple analogy is that of the surface of an expanding balloon. The balloon expands so fast that speed-of-light signals from distant parts never get to reach us, as the cumulative expansion over very large distances is effectively "faster than light". What I said in the previous paragraph still holds, though.
 
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  • #128
DrGreg said:
What I said in the previous paragraph still holds, though.


Would it be accurate to relate the curve of the balloon to the curvature of space? If we look back at the idea of the map maker trying to make a distant object on the Earth, would the expanding of space be like the Earth was growing/inflating while he was doing so?
 
  • #129
Bussani said:
Would it be accurate to relate the curve of the balloon to the curvature of space? If we look back at the idea of the map maker trying to make a distant object on the Earth, would the expanding of space be like the Earth was growing/inflating while he was doing so?
The two analogies I gave aren't really directly comparable. The "map of Earth" analogy is referring to spacetime, whereas the "expanding balloon" is referring to space. You can only take these analogies so far.
 
  • #130
DrGreg said:
According to general relativity (and ignoring the hypothetical, but very unlikely, possibility that tachyons might exist), nothing can overtake a photon that is traveling along the same route.

The numerical value of the speed of a photon depends on the coordinate system you measure it in. If you measure it locally, using a "local ruler" x and "local clock" t, you will always get dx/dt = c (=299792458 m/s exactly) no matter where you are in the Universe or how you are moving. But if you try to measure the speed of some light a distance away from yourself, you may well get a different numerical value. This is due to spacetime curvature. An analogy is that cartographers can accurately draw a scale map of an area a few miles across, but if you try to map a thousand miles of the Earth's surface on a flat piece of paper, the map could be very accurately to scale at the centre of the map, but distorted in angle or distance near the edges. This is what happens in relativity, long-distance measurements can get distorted.

As for the expanding Universe, the simple analogy is that of the surface of an expanding balloon. The balloon expands so fast that speed-of-light signals from distant parts never get to reach us, as the cumulative expansion over very large distances is effectively "faster than light". What I said in the previous paragraph still holds, though.

I like this answer the best. It combines what we DO know with what we don't and makes intuitive sense. Of course, SR and GR and all FR whatever references may just be part of a greater reality which we don't know just as Newton was part of the greater reality of relativity but who knows?
 
  • #131
DrGreg said:
The two analogies I gave aren't really directly comparable. The "map of Earth" analogy is referring to spacetime, whereas the "expanding balloon" is referring to space. You can only take these analogies so far.


Gotcha. Thanks.
 
  • #132
no object can travel faster than light because keeps increasing as we approach velocity of light beyond the speed of 0.999 c the mass becomes infinite so your appartus won't work galaxy are not moving faster than light the space which they are associated is expanding at unbelievable velocity relativity puts no constraint upon how fast the space could expands this is the reason why we the deep space is 42 billion light year deep atleast we can see this deep and universe is only 15 billion year old so the furthest we could see should be 15 bn not 42 and more.and such movement of space is the basis of FTL system like alcuiberre warp drive and slip string warp drive.no law breaks since matter is not traveling at the speed of light nor and information carrying signal only space is.sorry for getting a bit off topic
 
  • #133
kai0 said:
no object can travel faster than light because keeps increasing as we approach velocity of light beyond the speed of 0.999 c the mass becomes infinite so your appartus won't work galaxy are not moving faster than light the space which they are associated is expanding at unbelievable velocity relativity puts no constraint upon how fast the space could expands this is the reason why we the deep space is 42 billion light year deep atleast we can see this deep and universe is only 15 billion year old so the furthest we could see should be 15 bn not 42 and more.and such movement of space is the basis of FTL system like alcuiberre warp drive and slip string warp drive.no law breaks since matter is not traveling at the speed of light nor and information carrying signal only space is.sorry for getting a bit off topic

Would you please rewrite that?
 
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